CMB Secondary Anisotropies due to Galaxy Clusters

by Nabila Aghanim (IAS (Institut d’Astrophysique Spatiale) – Centre universitaire d’Orsay - Paris-Orasy - France)

Aula 3 (Dip. di Fisica - Edificio E. Fermi)

Aula 3

Dip. di Fisica - Edificio E. Fermi

Cosmic Microwave Background Secondary Anisotropies are becoming more and more important for future CMB experiments as they contribute to the both polarisation and temperature anisotropies at small angular scales. I will present some of the issues associated with the dominant secondary anistropies.